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The Giotto dust impact detection systemThe Giotto Dust Impact Detection System (DIDSY) consists of six independent subsystems to register the impact of all particulates of significant mass incident on the probe during the post-perihelion encounter with Comet Halley. Mounted on Giotto's front dust shield, the detectors will determine the mass spectrum of the dust, with a limiting sensitivity of 10 to the minus 17th power f, increasing to the largest grain masses encountered along Giotto's trajectory throught the cometary environment with an ultimate spatial resolution of 70 km. An additional detector is located on the rear shield to monitor dust particles that penetrate the from dust shield. An ambient plasma monitor measures the impact plasma generated by dust and gass impacts on the spacecraft.
Document ID
19860023008
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Mcdonnell, J. A. M.
(Kent Univ. Canterbury, United Kingdom)
Alexander, W. M.
(Baylor Univ. Waco, Tex., United States)
Burton, W. M.
(Rutherford High Energy Lab. Chilton, United Kingdom)
Bussoletti, E.
(Lecce Univ. Italy, United States)
Clark, D. H.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Evans, G. C.
(Kent Univ. Canterbury, United Kingdom)
Evans, S. T.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Firth, J. G.
(Rutherford High Energy Lab. Chilton, United Kingdom)
Grard, R. J. L.
(European Space Agency. European Space Research and Technology Center ESTEC, Noordwijk, Netherlands)
Gruen, E.
(Max-Planck-Inst. fuer Kernphysik Heidelberg, Germany)
Date Acquired
August 12, 2013
Publication Date
March 1, 1986
Publication Information
Publication: ESA The Giotto Mission: Its Scientific Investigations
Subject Category
Spacecraft Instrumentation
Accession Number
86N32480
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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